The idea behind the "The nature of Dark Matter at small scales"
workshop is to bring together people, working on observations
of the objects in the local halo, N-body simulations of
structure formation, Lyman-alpha analysis, weak gravitational
lensing, etc. The main goal is to understand what do we know
about the nature of DM at galaxy scales.

Each day of workshop will be devoted to one of these topics
(each presentation session followed the discussion)

What do we know about the nature of DM from observations
of Local halo?

What is the current state of the art of numerical
simulations of structure formation?

What can we learn about the nature of DM from cosmology
(Lyman-alpha forest observations, weak gravitational lensing,
etc.)

Acknowledgments
Financial support of this workshop was provided in part by
- Laboratory of Astroparticle Phsyics and Cosmology (APC, Paris)
- European Network of Theoretical Astroparticle Physics ILIAS/N6
(working group 2: Dark Matter and Related Studies) under contract number RII3-CT-2004-506222
- Europenian Science Foundation activity 'Computational Astrophysics and Cosmology'.